Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Non-thermal pressure support in X-COP galaxy clusters
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1805.00034.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-12T07:56:00.734481Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T12:52:10.461388Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation a08baed5-c692-433d-8657-8ab630cd4e7a · inbound
Beyond Self-Similarity: Reconciling X-Ray Scaling Relations in Galaxy Clusters and Groups cites this paper.
Beyond Self-Similarity: Reconciling X-Ray Scaling Relations in Galaxy Clusters and Groups Non-thermal pressure support in X-COP galaxy clusters
Reference 114
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T12:52:10.462537Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 4b56e75c-af4e-4858-85af-63db8822edf8 · inbound
Bulk vs. turbulent motions at the centres of galaxy clusters: AGN-driven turbulence according to TNG-Cluster cites this paper.
Bulk vs. turbulent motions at the centres of galaxy clusters: AGN-driven turbulence according to TNG-Cluster Non-thermal pressure support in X-COP galaxy clusters
Reference 62
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T05:01:39.464572Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation ef1b2c6b-b9fe-43b0-90d0-33c60224f4ba · inbound
The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \simeq 2$ protoclusters cites this paper.
The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \simeq 2$ protoclusters Non-thermal pressure support in X-COP galaxy clusters
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T07:56:00.734481Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.